Table 3
Stellar and wind parameters of models used to compare synthetic nitrogen line profiles from fastwind and cmfgen.
Model | Code | Teff | R ∗ | log g | log Q |
(K) | (R⊙) | (cgs) | |||
|
|||||
d2v | cmfgen | 46 100 | 11.4 | 4.01 | –12.43 |
E4740 | fastwind | 47 000 | 4.00 | –12.45 | |
d4v | cmfgen | 41 010 | 10.0 | 4.01 | –12.75 |
D4140 | fastwind | 41 000 | 4.00 | –12.80 | |
|
|||||
s2a | cmfgen | 44 700 | 19.6 | 3.79 | –11.99 |
F4540 | fastwind | 45 000 | 3.80 | –12.15 | |
s4a | cmfgen | 38 700 | 21.8 | 3.57 | –12.15 |
F3935 | fastwind | 39 000 | 3.50 | –12.15 |
Notes. The grid is a subset of the grid presented by Lenorzer et al. (2004). For details, see Paper I. Even entries provide those parameters from our fastwind grid models which reproduce best the H/He spectra from cmfgen. All models were calculated with vmic= 10 km s-1, and with four different nitrogen abundances, [N] = 7.78, 7.98, 8.38, 8.78. Wind strength parameter, Q, calculated in units of M⊙ yr-1, R⊙ and km s-1.
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